Enkelad (Enceladus) je prirodni Saturnov satelit kojeg je 1789. otkrio astronom William Herschel. Ime je dobio po gigantu Enkeladu iz starogrčke mitologije. Ovaj satelit ima drugo ime Saturn II.
Kratke činjenice Discovery, Discovered by ...
EnkeladEnceladus snimljen orbiterom Cassini, oktobar 2015. [a] |
|
Discovered by | William Herschel |
---|
|
Designation | Saturn II |
---|
Imenovan po | Ἐγκέλαδος Egkelados |
---|
Adjectives | Enceladean [1][2] |
---|
|
Semi-major axis | 7005237948000000000♠237.948 km[3] |
---|
Orbital period (sidereal) | 7006137021800000000♠1,370218 d[3] |
---|
Inclination | 0.009° (to Saturn's equator)[3] |
---|
|
Mean radius | 7003252100000000000♠252,1±0,2 km[4][5] (7002395000000000000♠0,0395 Earths, 7003145100000000000♠0,1451 Moons) |
---|
Surface gravity | 1.134 m/s2 (7002116000000000000♠0,0116 g) |
---|
Moment of inertia factor | 7003330500000000000♠0,3305±0,0025[6] |
---|
Escape velocity | 2.391 km/s (860.4 km/h)[3] |
---|
Synodic rotation period | Sinhrona |
---|
Axial tilt | 0 |
---|
Albedo | 7003137500000000000♠1,375±0,008 (geometrijski na 550 nm)[7] or 7001810000000000000♠0,81±0,04 (Bond)[8] |
---|
Surface temp. |
min |
mean |
max |
Kelvin[9] |
32.9 K |
75 K |
145 K |
Celsius |
−240 °C |
−198 °C |
−128 °C |
|
| 11.7[10] |
---|
|
Surface pressure | Trace, significant spatial variability[11][12] |
---|
Composition by volume | 91% vode pare 4% nitrogen 3.2% ugljen-dioksid 1.7% metan[13] |
---|
Zatvori
Enkelad obilazi Saturn svakih 32 h 53 m 7 s, ima prosječni prečnik od 498,9 km i masu od 8,6×1019 kg. Prosječna gustoća Enkelada iznosi 1,3 g/cm3. Mjerenja obavljena od strane svemirske letjelice Cassini-Huygens ookazala su da je ovaj satelit napravljen većinom od leda, vode i možda male količine kamena i metala.
Početkom 2006. NASA-ina letjelica Cassini snimila je erupcije gejzira na površini, vjerovatno sastavljene i od tekuće vode.
Postberg et al. "Plume and surface composition of Enceladus", p. 129–130, 148, 156; Lunine et al. "Future Exploration of Enceladus and Other Saturnian Moons", p. 454; in Schenk et al., eds. (2018) Enceladus and the Icy Moons of Saturn
- Brown, Robert H. (2006). "Composition and Physical Properties of Enceladus' Surface". Science. 311 (5766): 1425–1428.
- Castillo, Julie C. (2005). "26Al in the Saturnian System - New Interior Models for the Saturnian satellites". Eos Trans. AGU. 82 (52): Fall Meet. Suppl. Abstract P32A-01. Arhivirano s originala, 30. 9. 2007. Pristupljeno 3. 7. 2013.
- Castillo, J. C. (2006). "A New Understanding of the Internal Evolution of Saturnian Icy Satellites from Cassini Observations" (PDF). LPSC. XXXVII. Abstract 2200.
- Dougherty, M. K. (2006). "Identification of a Dynamic Atmosphere at Enceladus with the Cassini Magnetometer". Science. 311 (5766): 1406–1409.
- Hansen, Candice J. (2006). "Enceladus' Water Vapor Plume". Science. 311 (5766): 1422–1425.
- Matson, D.L. (2006). "Enceladus' Interior and Geysers - Possibility for Hydrothermal Geometry and N2 Production" (PDF). LPSC. XXXVII. Abstract 2219.
- Pappalardo, R.T. (2006). "Diapir-Induced Reorientation of Enceladus" (PDF). LPSC. XXXVII. Abstract 2113.
- Porco, C.C. (2006). "Cassini Observes the Active South Pole of Enceladus". Science. 311 (5766): 1393–1401.
- Rathbun, Julie A. (2005). "Enceladus' global geology as seen by Cassini ISS". Eos Trans. AGU. 82 (52): Fall Meet. Suppl. Abstract P32A-03. Arhivirano s originala, 4. 4. 2008. Pristupljeno 3. 7. 2013.
- Rothery, David A. (1999). Satellites of the Outer Planets: Worlds in their own right. Oxford University Press. ISBN 0-19-512555-X.
- Spahn, Frank (2006). "Cassini Dust Measurements at Enceladus and Implications for the Origin of the E Ring". Science. 311 (5766): 1416–1418.
- Spencer, J. R. (2006). "Cassini Encounters Enceladus: Background and the Discovery of a South Polar Hot Spot". Science. 311 (5766): 1401–1405.
- Turtle, Elizabeth et al. Enceladus, Curiouser and Curiouser: Observations by Cassini's Imaging Science Subsystem. Cassini CHARM Telecon. 28 April 2005. (Adobe Acrobat file).
- Verbiscer, Anne (2005). "The opposition surge of Enceladus: HST observations 338-1022 nm". Icarus. 173: 66–83. doi:10.1016/j.icarus.2004.05.001.
- Waite Jr., J. Hunter (2006). "Cassini Ion and Neutral Mass Spectrometer: Enceladus Plume Composition and Structure". Science. 311 (5766): 1419–1422.